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Lectures on natural philosophy
Structure of Space-Time
Christian Maes
(Dated: October 11, 2012)
As the world appears to possess spatial and temporal aspects, it is an important
question and even a central topic of natural philosophy to reflect on the nature of
that space-time arena.
I. NATURAL PHILOSOPHY
Natural philosophy is a philosophical reflection on nature, and more in particular it is
the study of foundational aspects of the natural sciences. It is mostly developed in the
study of philosophy of physics, but its ambition today also reaches aspects of biology,
chemistry, computer science etc. The intellectual tradition started in Greece in the Milesian
school founded in the 6th century BC, flourishing in the pre-socratic philosophy and in
the Hellenistic period with Archimedes as culminating figure and father of mathematical
physics. From there, scientific culture was mostly preserved in the Arabic and Muslim
world. A new age will only start with the work of Galileo and Newton, which also marks
the beginning of classical mechanics in the 17th century. Newton still writes about the
mathematical principles of natural philosophy, but in the next centuries, the term itself
(natural philosophy) must make room for the nomenclature of more specialized scientific
and philosophical disciplines.
The Greek miracle refers to the rather rapid birth (6th-4th century BC) and develop-
ment of a scientific culture in ancient Greek, steered by a new ambition of explaining nature
through nature. That intellectual project was mostly speculative and theoretical, but dif-
fered from Babylonian or Egyptian efforts that mostly dealt with data-collection and their
fitting with simple models. The Greek nature-philosophers reached much further. Here we
have philosophers discussing nature devoid of supernatural causes or of mythical origins,
presenting the being and working of nature in terms of mechanisms and causes that refer to
methodologically observable quantities. A second meaning of the word nature is found in
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natural motion (to be distinguished from forced motion). That is decided by the
structure of space: an untouched sublunar world would segregate in earth, then water, then
air, then fire. We thus have a spherical rocky earth covered by oceans and air. There is a
geometrically privileged center and the universe is a sphere around it. The fifth nature
(the quintessence) is called the aether, whose natural motion is uniform circular around the
center. That motion is realized by the sphere of fixed stars, turning around with perfect
regularity and defining time itself. Astronomers task for the coming centuries would be to
understand the motion of the sun, the moon and the planets as a combination of circular
motions.
The influence of Aristotles way of thinking and of his world view on Western thought
cannot be overestimated, especially after its incorporation in a Christian theology. The
notion of natural place has in general brought about the idea of natural (immanent)
justice and natural living, i.e., according to a given or imposed structure and order of
the universe.
III. GALILEIS NEW SCIENCE
There is no perfect, unchanging sphere around the center of the universe. The outlook
on how the universe looks like changes drastically in the 15th-16th century. To start with
the solar system, GG adopted Copernicus heliocentric hypothesis, and thought of planet
Earth very much as being just a planet. In fact, his discoveries with the telescope helped
to revolutionize astronomy, to accept the Copernican system.
Galileo Galilei (born in 1564, dying in 1642) was very much inspired by Archimedes and
very much natural philosopher, astronomer, and mathematician. Besides to the sciences
of motion, astronomy, and material science, he also contributed to the development of the
scientific method. There, systematic experiment joined with mathematical (geometric) and
quantitative analysis, rejecting teleological arguments.
The main discovery on motion was to unite motion with rest. Before GG motion was
ontologically different from rest. With GG motion is as natural as rest. Galileo reasoned
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that moving objects eventually stop because of a force called friction. The more systematic
development is however Newtons work. For our discussion, two further studies are impor-
tant, 1) free fall, 2) relativity principle.
ad 1) Galileo discovers that the distance fallen is proportional to the square of the time
it has been falling. He uses balls rolling on inclined planes to show that different weights
fall with the same acceleration. Regardless of the angle at which the planes are oriented,
the final height almost always equals the initial height. Reducing the slope of the opposite
incline, the ball rolls a further distance in order to reach that original height. Taking the
elevation at nearly a 0-degree angle, the ball would roll almost forever, like making an effort
to reach the original height. And if the opposing incline was not even inclined at all (that
is, if it were oriented along the horizontal), then ... an object in motion would continue in
motion. In fact, GG thought it would continue in circular motion.
ad 2) Relativity: GG emphasizes the relativity of motion, and the invariance of natural laws
under uniform straight motion.
IV. NEWTONS PROGRAMME
Isaac Newton (born in 1642 or in 1643 depending on the calendar, dies in 1727) was the
culminating figure of the scientific revolution of the 17th century. His Philosophiae Naturalis
Principia Mathematica of 1687 is one of the most important single works in the history of
modern science.
A. First law
Every body preseveres in its state either of rest or of uniform motion in a straight line,
except insofar as it is complelled to change its state by impressed forces.It means every body, apples and moons. Unification: No fundamental diversity. The
force that maintains the moon in orbit about the earth is precisely the same force that
causes an apple to fall from a tree.
No natural motion is ascribed to a body; in fact every body has an innate tendency to
maintainits state of motion. No need for special points in the universe. Rather, the arena
of motion is absolute space. That space has a structure to give meaning to the notion of
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rest and uniform motion in a straight line.
Space and geometry is Euclidean. Absolute space is 3-dimensional E3, infinite in all
directions with the structure of pencil, straightedge and compass. That is to say, there is a
notion of topology so that we know what we mean by continuous curves. There is a notion
of affinity so that we know what we mean by straight lines and there is a notion of metric
so that we can estimate distances. We also need an absolute time ot measure time, which
goes forward.
Newton believes that this 3-dimensional space exists at every moment of time, and
moreover that identically the same points of space persist through time. For a body to be
resting it means to remain in the same points of absolute space. Same thing for uniform
motion in a straight line.
Newton understands that these persisting parts of absolute motion cannot be perceived
by our senses. What we can observe are the relative positions, or the relative times. Of
course the belief in absolute space is not strange, but Newton will appeal to experiment to
try to prove its existence.
B. Second law
The First law formulates the state of motion of every body when there is no external
force: it is either rest or uniform straight motion in and with respect to absolute space.
That is however insufficient to account for the world where bodies are almost never seen in
uniform motion. In the Second law, Newton launches his programme on forces:
The change in motion is proportional to the impressed motive force, and is made along the
straight line on which the force is impressed.
By the first law, we know what a change of motion means. From the second law we say
that to keep a body say in uniform circular motion, there must be always a force (the
centripetal force). The moon is attracted to the earth by such a force, gravity.
Newton goes on by noticing that the very observation of forces thus means that there is
change of motion, hence absolute space. More precisely he is using the famous bucket
experiment to prove the existence of absolute space. In an otherwise empty space, two
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spheres connected by a cord and rotating around their common center of gravity can be
considered as rotating with respect to absolute space. There is absolute rotation, hence
absolute space and time.
If a vessel, hung by a long cord, is so often turned about that the cord is strongly twisted,
then filled with water, and held at rest together with the water; after, by the sudden action
of another force, it is whirled about in the contrary way, and while the cord is untwisting
itself, the vessel continues for some time this motion; the surface of the water will at first
be plain, as before the vessel began to move; but the vessel by gradually communicating its
motion to the water, will make it begin sensibly to revolve, and recede by little and little,
and ascend to the sides of the vessel, forming itself into a concave figure...This ascent of the
water shows its endeavour to recede from the axis of its motion; and the true and absolute
circular motion of the water, which is here directly contrary to the relative, discovers itself,
and may be measured by this endeavour. ... And therefore, this endeavour does not depend
upon any translation of the water in respect to ambient bodies, nor can true circular motion
be defined by such translation. ...; but relative motions...are altogether destitute of any real
effect. ...It is indeed a matter of great difficulty to discover, and effectually to distinguish,
the true motions of particular bodies from the apparent; because the parts of that immovable
space in which these motions are performed, do by no means come under the observations
of our senses. Isaac Newton; Principia, Book 1: Scholium.
The rotating bucket argument demonstrates that true rotational motion cannot be defined
as the relative rotation of the body with respect to the immediately surrounding bodies. In
general, true motion and rest cannot be defined as special instances of motion or rest relative
to other bodies, but instead can be defined only by reference to absolute space. Alternatively,
these experiments provide an operational definition of what is meant by absolute rotation,
and do not pretend to address the question of rotation relative to what?.
C. Absolute space
Absolute, true and mathematical time, of itself, and from its own nature flows equably
without regard to anything external, and by another name is called duration: relative, ap-
parent and common time, is some sensible and external (whether accurate or unequable)
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measure of duration by the means of motion, which is commonly used instead of true time
...
Absolute space, in its own nature, without regard to anything external, remains always
similar and immovable. Relative space is some movable dimension or measure of the
absolute spaces; which our senses determine by its position to bodies: and which is vulgarly
taken for immovable space ... Absolute motion is the translation of a body from one absolute
place into another: and relative motion, the translation from one relative place into another.
We have seen already above how absolute space very naturally enters as the arena of
motion according to Newton. Space has an Euclidean structure, but not much of that is
used for the dynamics itself. Space is infinite, totally homogeneous and symmetric and
many debates have since long been held on how anything can occur in such a universe;
there is too much freedom and no particular place can be taken. Other objections are the
metaphysical nature of space and time. To the latter, we can add the Galilean invariance
principle, which slightly but essentially changes the structure of Newtonian space-time into
Galilean space-time. It is a way to eliminate unobservable behavior.
For Newton, the trajectories of bodies in absolute uniform motion in a straight line
through absolute space are represented by straight lines in a space-time diagram. Putting
a force on an object curves the world-line in the direction of the force. Going to a Galilean
picture, we only make differences between straight and curved trajectories. We no longer
speak about space and time separately, but about events happening in space-time, without
need to identify spatial points throughout time.
D. Determinism
We may regard the present state of the universe as the effect of its past and the cause
of its future. An intellect which at a certain moment would know all forces that set nature
in motion, and all positions of all items of which nature is composed, if this intellect were
also vast enough to submit these data to analysis, it would embrace in a single formula the
movements of the greatest bodies of the universe and those of the tiniest atom; for such an
intellect nothing would be uncertain and the future just like the past would be present before
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its eyes. Pierre Simon Laplace, A Philosophical Essay on Probabilities.
E. Conservation laws
Classical mechanics introduces the concept of energy as conserved over Newtonian tra-
jectories.
F. Gravity
Newton discovers the universal law of gravitation.
I have not as yet been able to discover the reason for these properties of gravity from
phenomena, and I do not feign hypotheses.
That one body may act upon another at a distance through a vacuum without the mediation
of anything else, by and through which their action and force may be conveyed from one
another, is to me so great an absurdity that, I believe, no man who has in philosophic
matters a competent faculty of thinking could ever fall into it.